The LIGO Scientific Collaboration and the Virgo Collaboration report:
We identified the compact binary merger candidate S190602aq during
real-time processing of data from LIGO Hanford Observatory (H1), LIGO
Livingston Observatory (L1), and Virgo Observatory (V1) at 2019-06-02
17:59:27.089 UTC (GPS time: 1243533585.089). The candidate was found
by the PyCBC Live , CWB , SPIIR , GstLAL , and MBTAOnline
 analysis pipelines.
S190602aq is an event of interest because its false alarm rate, as
estimated by the online analysis, is 1.9e-09 Hz, or about one in 16
years. The event's properties can be found at this URL:
The classification of the GW signal, in order of descending
probability, is BBH (>99%), Terrestrial (<1%), BNS (<1%), NSBH (<1%),
or MassGap (<1%).
Assuming the candidate is astrophysical in origin, there is strong
evidence against the lighter compact object having a mass < 3 solar
masses (HasNS: <1%). Using the masses and spins inferred from the
signal, there is strong evidence against matter outside the final
compact object (HasRemnant: <1%).
One skymap is available at this time and can be retrieved from the
GraceDB event page:
* bayestar.fits.gz, an updated localization generated by BAYESTAR
, distributed via GCN notice about 6 minutes after the candidate
For the bayestar.fits.gz skymap, the 90% credible region is 1172 deg2.
Marginalized over the whole sky, the a posteriori luminosity distance
estimate is 797 +/- 238 Mpc (a posteriori mean +/- standard
For further information about analysis methodology and the contents of
this alert, refer to the LIGO/Virgo Public Alerts User Guide
 Nitz et al. PRD 98, 024050 (2018)
 Klimenko et al. PRD 93, 042004 (2016)
 Qi Chu, PhD Thesis, The University of Western Australia (2017)
 Messick et al. PRD 95, 042001 (2017)
 Adams et al. CQG 33, 175012 (2016)
 Singer & Price PRD 93, 024013 (2016)